Thermally Pulsing AGB Models of Intermediate Mass Stars

Details Thermally Pulsing AGB Models of Intermediate Mass Stars Thermally Pulsing AGB Models of Intermediate Mass Stars

1999-12-20

arxiv.org/abs/astro-ph/9912426v1

Astronomy and Astrophysics

Astrophysics

9 pages, 9 figures (memsait.sty, epsf.sty) contribution to the workshop "The Changes in Abundances in Asymptotic Giant Branch

Scientific paper

We present a set of models of AGB stars with initial mass larger than 5 Mo as
obtained with the FRANEC code. It includes models of Z=0.02 and Z=0.001, with
and without mass loss.

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